ALT A large galaxy takes up the entirety of the image. The core is mostly bright white, but there are also swirling, detailed structures that resemble water circling a drain. There is white and light blue colored dust that emanates from the core’s center, but it is tightly contained to the core. The rings are wispy and highlight filaments of dust around cavernous black bubbles. The dust in the outer rings contains dots that are navy blue, pinkish, reddish, and white.

ALT A large galaxy takes up the entirety of the image. Six reddish diffraction spikes extend from the core. The spiral arms of the galaxy outstretch to the upper left and the lower right. The arms are wispy and highlight filaments of dust around cavernous black bubbles. That dust in the outer rings contains diffuse dots that are navy blue, pinkish, reddish, and white.

ALT A large spiral galaxy takes up the entirety of the image, with the lower right portion of the galaxy’s spiral arms extending out of frame. The core of the galaxy i

ALT A Webb image of the central region of the Chamaeleon I dark molecular cloud, which resides 630 light-years away. This image primarily shows blue smoky wisps on a dark background. The left top side additionally features orange and white wisps. Just below them are four bright points of light. Three are orange and one is a mix of white and orange. Each of these points have Webb’s signature 8-point diffraction spikes emanating around them in long, thick orange lines, so that they look like huge snowflakes. Scattered throughout the image are distant stars or galaxies in shades of red, orange and blue, seen as tiny blobs.